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dc.date.accessioned | 2022-09-26T13:16:56Z | |
dc.date.available | 2022-09-26T13:16:56Z | |
dc.date.issued | 1990 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/142717 | |
dc.description.abstract | The asteroid 423 Diotima was observed photoelectrically in V filter during October 1987 at Observatorio Municipal de Mercedes. The synodic rotational period and amplitude obtained are: P=4.626 ± 0.002 hours and Δm=0.196 ± 0.014. The values confirm the solution proposed by Zappala et al. (1985) to the ambiguity presented in previous determinations of the rotational period and convert this asteroid in a peculiar object. | en |
dc.language | es | es |
dc.subject | Galaxia | es |
dc.title | Rotation period and light curve of asteroid 423 Diotima | en |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Gil-Hutton, Ricardo Alfredo | es |
sedici.subject.materias | Astronomía | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Asociación Argentina de Astronomía | es |
sedici.subtype | Comunicacion | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.relation.journalTitle | Boletín de la Asociación Argentina de Astronomía | es |
sedici.relation.journalVolumeAndIssue | no. 36 | es |
dc.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |